Decay of 23Ne

R. Moreh; J. Balderman; Y. Gozez

doi:10.1016/0375-9474(68)90740-9

Decay of ²³Ne

R. Moreh, J. Balderman, Y. Gozez

Research output: Contribution to journal › Article › peer-review

7 Scopus citations

Abstract

The gamma radiation following the decay of ²³Ne produced by ²²Ne(n, γ) reaction has been studied using Ge(Li) detectors. No indications were found for levels at 2.285, 2.405 and 2.870 MeV excitation reported by Lancman et al.

Original language	English
Pages (from-to)	236-240
Number of pages	5
Journal	Nuclear Physics A
Volume	107
Issue number	1
DOIs	https://doi.org/10.1016/0375-9474(68)90740-9
State	Published - 8 Jan 1968
Externally published	Yes

Keywords

Radioactivity

ASJC Scopus subject areas

Nuclear and High Energy Physics

Access to Document

10.1016/0375-9474(68)90740-9

Cite this

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title = "Decay of 23Ne",

abstract = "The gamma radiation following the decay of 23Ne produced by 22Ne(n, γ) reaction has been studied using Ge(Li) detectors. No indications were found for levels at 2.285, 2.405 and 2.870 MeV excitation reported by Lancman et al.",

keywords = "Radioactivity",

author = "R. Moreh and J. Balderman and Y. Gozez",

year = "1968",

month = jan,

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doi = "10.1016/0375-9474(68)90740-9",

language = "English",

volume = "107",

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journal = "Nuclear Physics A",

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AU - Moreh, R.

AU - Balderman, J.

AU - Gozez, Y.

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N2 - The gamma radiation following the decay of 23Ne produced by 22Ne(n, γ) reaction has been studied using Ge(Li) detectors. No indications were found for levels at 2.285, 2.405 and 2.870 MeV excitation reported by Lancman et al.

AB - The gamma radiation following the decay of 23Ne produced by 22Ne(n, γ) reaction has been studied using Ge(Li) detectors. No indications were found for levels at 2.285, 2.405 and 2.870 MeV excitation reported by Lancman et al.

KW - Radioactivity

UR - http://www.scopus.com/inward/record.url?scp=33846394016&partnerID=8YFLogxK

U2 - 10.1016/0375-9474(68)90740-9

DO - 10.1016/0375-9474(68)90740-9

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JO - Nuclear Physics A

JF - Nuclear Physics A

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